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Kes 69, 3C 396, and 3C 400.2 are mixed-morphology (MM) Galactic supernovaremnants (SNRs), where Kes 69 and 3C 396 are interacting with molecular clouds(MCs). Previous X-ray studies showed that the emission from these SNRs isthermal. It has been suggested that MM SNRs interacting with MCs are potentialcandidates for recombining plasma (RP) in X-rays and hadronic gamma-rayemission. Recently, Chandra observations revealed signs of RP in 3C 400.2. Ourpreliminary analyses show that the X-ray emission of NW and SE region of 3C400.2 arises from recombining plasma. We detected GeV gamma-ray emission fromKes 69 and 3C 396 above 5$\sigma$.

Investigating the X-ray and Gamma-ray Properties of the Galactic Supernova Remnants Kes 69, 3C 396, 3C 400.2